137 research outputs found

    Cabibbo suppressed decays and the Ξc+\Xi_{c}^{+} lifetime

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    The problem of the Ξc+\Xi_{c}^{+} lifetime is considered in the framework of {\em Heavy-Quark Expansion} and SU(3)flavorSU(3)_{flavor} symmetry. The lifetime of Ξc+\Xi_{c}^{+} is expressed in terms of measurable inclusive quantities of the other two charmed baryons belonging to the same SU(3)flavorSU(3)_{flavor} multiplet in a model-independent way. In such a treatment, inclusive decay rates of singly Cabibbo suppressed decay modes have a prominent role. An analogous approach is applied to the multiplet of charmed mesons yielding interesting predictions on Ds+D_{s}^{+} properties. The results obtained indicate that a more precise measurement of inclusive decay quantities of some charmed hadrons (such as Λc+\Lambda_{c}^{+}) that are more amenable to experiment can contribute significantly to our understanding of decay properties of other charmed hadrons (such as Ξc+\Xi_{c}^{+}) where discrepancies or ambiguities exist.Comment: 9 pages, revtex4; certain improvements in text as suggested by the referee, acknowledgement changed; version to appear in Phys. Rev.

    Perturbative QCD Fragmentation Functions for Production of P-wave Mesons with Charm and Beauty

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    We calculate the leading order QCD fragmentation functions for the production of PP-wave charmed beauty mesons. Long-distance effects are factored into two nonperturbative parameters: the derivative of the radial wavefunction at the origin and a second parameter related to the probability for a (bˉc)(\bar b c) heavy quark pair that is produced in a color-octet SS-wave state to form a color-singlet PP-wave bound state. The four 2P2P states and those 3P3P states which lie below the BDBD flavor threshold eventually all decay into the 1S1S ground state BcB_c through hadronic cascades or by emitting photons. The total fragmentation probabilities for production of the 1S1S ground state BcB_c from the cascades of the 2P2P and 3P3P states are about 1.7×1041.7 \times 10^{-4} and 2.3×1042.3 \times 10^{-4} respectively. Thus the direct production of the PP-wave states via fragmentation may account for a significant fraction of the inclusive production rate of the BcB_c at large transverse momentum in high energy colliders. Our analytic results for the PP-wave fragmentation functions disagree with those obtained earlier in the literature.Comment: 31 pages, Latex file, 1 figure (postscript file appended at the end

    Lifetimes of Heavy-Flavour Hadrons -- Whence and Whither?

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    A theoretical treatment for the weak decays of heavy-flavour hadrons has been developed that is genuinely based on QCD. Its methodology as it applies to total lifetimes and the underlying theoretical issues are sketched. Predictions are compared with present data. One discrepancy emerges: the beauty baryon lifetime appears to be significantly shorter than expected. The ramifications of those findings are analyzed in detail.Comment: 15 pages, no figures, LATEX, two references added and new information concerning a lower charm content in B decays incorporate

    A Tracker Solution for a Holographic Dark Energy Model

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    We investigate a kind of holographic dark energy model with the future event horizon the IR cutoff and the equation of state -1. In this model, the constraint on the equation of state automatically specifies an interaction between matter and dark energy. With this interaction included, an accelerating expansion is obtained as well as the transition from deceleration to acceleration. It is found that there exists a stable tracker solution for the numerical parameter d>1d>1, and dd smaller than one will not lead to a physical solution. This model provides another possible phenomenological framework to alleviate the cosmological coincidence problem in the context of holographic dark energy. Some properties of the evolution which are relevant to cosmological parameters are also discussed.Comment: 10 pages, 3 figures; accepted for publication in Int.J.Mod.Phys.

    Renormalization-group running cosmologies - a scale-setting procedure

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    For cosmologies including scale dependence of both the cosmological and the gravitational constant, an additional consistency condition dictated by the Bianchi identities emerges, even if the energy-momentum tensor of ordinary matter stays individually conserved. For renormalization-group (RG) approaches it is shown that such a consistency relation ineluctably fixes the RG scale (which may have an explicit as well as an implicit time dependence), provided that the solutions of the RG equation for both quantities are known. Hence, contrary to the procedures employed in the recent literature, we argue that there is no more freedom in identification of the RG scale in terms of the cosmic time in such cosmologies. We carefully set the RG scale for the RG evolution phrased in a quantum gravity framework based on the hypothetical existence of an infrared (IR) fixed point, for the perturbative regime within the same framework, as well as for an evolution within quantum field theory (QFT) in a curved background. In the latter case, the implications of the scale setting for the particle spectrum are also briefly discussed.Comment: v1:15 pages, 1 figure. v2: references added. v3: discussion of the physical interpretation of the scale-setting procedure added. v4: discussions added. Version to appear in Phys. Rev.

    OSOBA SA PSIHIČKIM POREMEĆAJEM POČINITELJ PROTUPRAVNIH DJELA U ZATVORSKOM SUSTAVU - PRIKAZ SLUČAJA I PREGLED ZAKONSKIH PROPISA KOJI REGULIRAJU POSTUPANJE

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    Prikazan je slučaj bolesnika hospitaliziranog na Odjelu forenzičke psihijatrije Zatvorske bolnice u Zagrebu pod dijagnozama Trajna promjena ličnosti nakon katastrofičnog događaja (proizašla iz kroničnog PTSP) i Ovisnost o alkoholu, koji je uz kaznu zatvora imao izrečenu sigurnosnu mjeru obveznog psihijatrijskog liječenja po čl. 68. novog Kaznenog zakona (član 75. starog KZ-a). U sklopu pojedinačnog programa izvršavanja kazne zatvora bolesnik je uključen u bio-psiho-socijalni model liječenja i rehabilitacije. U radu je prikazan i osvrt na zakonom propisane postupke prema osobama sa psihičkim poremećajem koje su počinile neko protupravno djelo. Ako je osoba počinila lakše protupravno djelo procesuira se po Prekršajnom zakonu, Zakonu o zaštiti od nasilja u obitelji i Zakonu o zaštiti osoba sa psihičkim poremećajem, koje sankcije se provode na slobodi u forenzičnim ambulantama javnog zdravstva ili psihijatrijskim odjelima bolnica javnog zdravstva. U slučajevima kada je osoba počinila teže kazneno djelo sudski se postupci provode u skladu s odredbama Zakona o kaznenom postupku, Kaznenog zakona i Zakona o zaštiti osoba s psihičkim poremećajem, a tretman se provodi unutar zatvorskog sustava, ako je osoba bitno smanjeno ubrojiva i uz kaznu zatvora joj je izrečena sigurnosna mjera obveznog psihijatrijskog liječenja (čl.68. KZ/11) ili liječenja od ovisnosti (čl. 69. KZ/11), odnosno na forenzičkim odjelima javnog zdravstva, ako se radi o neubrojivoj osobi koja je zbog svog psihičkog poremećaja opasna za okolinu

    Four-quark Operators Relevant to B Meson Lifetimes from QCD Sum Rules

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    At the order of 1/m_b^3, the B meson lifetimes are controlled by the hadronic matrix elements of some four-quark operators. The nonfactorizable magnitudes of these four-quark operator matrix elements are analyzed by QCD sum rules in the framework of heavy quark effective theory. The vacuum saturation for color-singlet four-quark operators is justified at hadronic scale, and the nonfactorizable effect is at a few percent level. However for color-octet four-quark operators, the vacuum saturation is violated sizably that the nonfactorizable effect cannot be neglected for the B meson lifetimes. The implication to the extraction of some of the parameters from B decays is discussed. The B meson lifetime ratio is predicted as \tau(B^-)/\tau(B^0)=1.09\pm 0.02. However, the experimental result of the lifetime ratio \tau(\Lambda_b)/\tau(B^0) still cannot be explained.Comment: 20 pages, latex, 6 figures, discussion on non-factorizable effect of the four-quark condensate added, to appear in Phys. Rev. D57 (1998

    Hadronic Production of Doubly Charmed Baryons via Charm Exitation in Proton

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    The production of baryons containing two charmed quarks Xi_cc in hadronic interactions at high energies and large transverse momenta is considered. It is supposed, that Xi_cc-baryon is formed during a non-perturbative fragmentation of the (cc)-diquark, which was produced in the hard process of cc-quark scattering from the colliding protons: c+c -> (cc) +g. It is shown that such mechanism enhances the expected doubly charmed baryon production cross section on Tevatron and LHC colliders approximately 2 times in contrast to predictions, obtained in the model of gluon - gluon production of (cc)-diquarks in the leading order of perturbative QCD.Comment: LaTeX2e, 13 pages plus 4 fig. using revtex4.sty, epsfig.sty. Talk was presented at International Seminar on Physics of Fundamental Interactions in ITEP, Moscow, Russia, November 27 - December 1, 200

    P-Wave Charmonium Production in B-Meson Decays

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    We calculate the decay rates of BB mesons into P-wave charmonium states using new factorization formulas that are valid to leading order in the relative velocity of the charmed quark and antiquark and to all orders in the running coupling constant of QCD. We express the production rates for all four P states in terms of two nonperturbative parameters, the derivative of the wavefunction at the origin and another parameter related to the probability for a charmed-quark-antiquark pair in a color-octet S-wave state to radiate a soft gluon and form a P-wave bound state. Using existing data on BB meson decays into χc1\chi_{c1} to estimate the color-octet parameter, we find that the color-octet mechanism may account for a significant fraction of the χc1\chi_{c1} production rate and that BB mesons should decay into χc2\chi_{c2} at a similar rate.Comment: 14 page

    Holographic Dark Energy Like in f(R)f(R) Gravity

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    We investigate the corresponding relation between f(R)f(R) gravity and holographic dark energy. We introduce a kind of energy density from f(R)f(R) which has role of the same as holographic dark energy. We obtain the differential equation that specify the evolution of the introduced energy density parameter based on varying gravitational constant. We find out a relation for the equation of state parameter to low redshifts which containing varying GG correction.Comment: 10 page
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